K2 Ultracool Dwarfs Survey – VI. White light superflares observed on an L5 dwarf and flare rates of L dwarfs

@article{Paudel2020K2UD,
  title={K2 Ultracool Dwarfs Survey – VI. White light superflares observed on an L5 dwarf and flare rates of L dwarfs},
  author={Rishi R. Paudel and John E. Gizis and D. J. Mullan and Sarah J. Schmidt and A. J. Burgasser and P. K. G. Williams},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2020},
  volume={494},
  pages={5751-5760}
}
Kepler K2 long cadence data are used to study white light flares in a sample of 45 L dwarfs. We identified 11 flares on 9 L dwarfs with equivalent durations of (1.3 - 198) hr and total (UV/optical/IR) energies of $\geq$0.9 $\times$ 10$^{32}$ erg. Two superflares with energies of $>$10$^{33}$ erg were detected on an L5 dwarf: this is the coolest object so far on which flares have been identified. The larger superflare on this L5 dwarf has an energy of 4.6$\times$ 10$^{34}$ ergs and an amplitude… 

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